Induced gravity from gauge theories
R. F. Sobreiro, A. A. Tomaz, V. J. Vasquez Otoya

TL;DR
This paper explores how certain four-dimensional gauge theories can potentially describe quantum gravity, leading to emergent Riemann-Cartan geometry and linking physical constants to the theory's dynamics.
Contribution
It proposes a framework where gauge theories of de Sitter groups can give rise to gravity and relate quantum field theory concepts to spacetime geometry.
Findings
Emergence of Riemann-Cartan gravity from gauge theories
Identification of geometric spacetime observables with physical quantities
Determination of Newton and cosmological constants from the theory's dynamics
Abstract
We discuss the possibility of a class of gauge theories, in four Euclidean dimensions, to describe gravity at quantum level. The requirement is that, at low energies, these theories can be identified with gravity as a geometrodynamical theory. Specifically, we deal with de Sitter-type groups and show that a Riemann-Cartan first order gravity emerges. An analogy with quantum chromodynamics is also formulated. Under this analogy it is possible to associate a soft BRST breaking to a continuous deformation between both sectors of the theory, namely, ultraviolet and infrared. Moreover, instead of hadrons and glueballs, the physical observables are identified with the geometric properties of spacetime. Furthermore, Newton and cosmological constants can be determined from the dynamical content of the theory.
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